MAGRINI, Laura, Sofia RANDICH, Manuala ZOCCALI, Lucie JÍLKOVÁ, Giovanni CARRARO, Daniele GALLI, Enrico MAIORCA and Maurizio BUSSO. Open clusters towards the Galactic centre: chemistry and dynamics. A VLT spectroscopic study of NGC 6192, NGC 6404, NGC 6583. Astronomy and Astrophysics. Les Ulis Cedex, France: EDP Sciences, 2010, vol. 523, No 1, p. 11-27, 16 pp. ISSN 0004-6361. Available from: https://dx.doi.org/10.1051/0004-6361/201015395.
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Basic information
Original name Open clusters towards the Galactic centre: chemistry and dynamics. A VLT spectroscopic study of NGC 6192, NGC 6404, NGC 6583
Name in Czech Otevrene hvezdokupy smerem k centru Galaxie: chemicke slozeni a dynamika, VLT spektroskopie NGC 6192, NGC 6404, NGC 6583
Authors MAGRINI, Laura (380 Italy, guarantor), Sofia RANDICH (380 Italy), Manuala ZOCCALI (380 Italy), Lucie JÍLKOVÁ (203 Czech Republic, belonging to the institution), Giovanni CARRARO (380 Italy), Daniele GALLI (380 Italy), Enrico MAIORCA (380 Italy) and Maurizio BUSSO (380 Italy).
Edition Astronomy and Astrophysics, Les Ulis Cedex, France, EDP Sciences, 2010, 0004-6361.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher France
Confidentiality degree is not subject to a state or trade secret
WWW URL
Impact factor Impact factor: 4.425
RIV identification code RIV/00216224:14310/10:00049707
Organization unit Faculty of Science
Doi http://dx.doi.org/10.1051/0004-6361/201015395
UT WoS 000285346600015
Keywords in English Galaxy open clusters NGC 6192 NGC 6404 NGC 6583
Tags AKb, rivok
Tags Reviewed
Changed by Changed by: Mgr. Lucie Jílková, Ph.D., učo 106183. Changed: 15/3/2013 13:06.
Abstract
We present new high-resolution spectroscopic observations obtained with FLAMES and the fiber link to UVES at VLT of three open clusters (OCs) located within 7 kpc from the Galactic centre (GC): NGC 6192, NGC 6404, NGC 6583. We also present new orbit determination for all OCs with Galactocentric distances (RGC) < 8 kpc and metallicity from high-resolution spectroscopy.
Links
GD205/08/H005, research and development projectName: Fyzika Slunce, hvězd a hvězdných soustav
Investor: Czech Science Foundation, Physics of Sun, stars, and stellar systems
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